Spiral galaxies, including the Milky Way, have large-scale magnetic fields with significant
energy densities. The dominant theory attributes these magnetic fields to a large-scale …

Context. Magnetic fields permeate the diffuse interstellar medium (ISM) of the Milky Way,
and are essential to explain the dynamical evolution and current shape of the Galaxy …

Magnetic fields are now widely recognized as critical at many scales to galactic dynamics
and structure, including multiphase pressure balance, dust processing, and star formation …

The magnetic fields in our Milky Way can be revealed by the distribution of Faraday rotation
measures (RMs) of radio sources behind the Galaxy and of radio pulsars inside the Galaxy …

We present the continued analysis of polarization and Faraday rotation for the supernova
remnants (SNRs) G46. 8− 0.3 and G39. 2− 0.3 in L-band (1–2 GHz) radio continuum in The …

We develop a new method for studying the Galactic magnetic field along the spiral arms
using pulsar Faraday rotation measures (RMs). Our new technique accounts for the dot …

A direct consequence of Faraday rotation is that the polarized radio sky does not resemble
the total intensity sky at long wavelengths. We analyze G137+ 7, which is undetectable in …

Context. Dusty magnetized structures observable in the far-infrared (FIR) at high Galactic
latitudes are ubiquitous and found to be closely related to HI filaments with coherent velocity …

Plasma lensing displays interesting characteristics that set it apart from gravitational lensing.
The magnetized medium induces birefringence in the two polarization modes. As the …

Context. During the first four all-sky surveys eRASS: 4, which was carried out from
December 2019 to 2021, the extended Roentgen Survey with an Imaging Telescope Array …